Inverse problem: Reconstruction of modified gravity action in Palatini formalism by Supernova Type Ia data
arXiv:0912.2410 · doi:10.1103/PhysRevD.80.124049
Abstract
We introduce in gravity--Palatini formalism the method of inverse problem to extract the action from the expansion history of the universe. First, we use an ansatz for the scale factor and apply the inverse method to derive an appropriate action for the gravity. In the second step we use the Supernova Type Ia data set from the Union sample and obtain a smoothed function for the Hubble parameter up to the redshift~1.7. We apply the smoothed Hubble parameter in the inverse approach and reconstruct the corresponding action in gravity. In the next step we investigate the viability of reconstruction method, doing a Monte-Carlo simulation we generate synthetic SNIa data with the quality of union sample and show that roughly more than 1500 SNIa data is essential to reconstruct correct action. Finally with the enough SNIa data, we propose two diagnosis in order to distinguish between the CDM model and an alternative theory for the acceleration of the universe.
8 pages, 8 figures, accepted in Phys. Rev. D
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Cited by in corpus (15)
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- Hamiltonian Formulation of Palatini f(R) theories a la Brans-Dicke
- Kinematic model-independent reconstruction of Palatini cosmology
- General slow-roll inflation in gravity under the Palatini approach
- Testing f(R) gravity with the simulated data of gravitational waves from the Einstein Telescope
- Reconstructing cosmic acceleration from modified and non-minimal gravity: The Yang-Mills case
- Loop Quantum Cosmology Matter Bounce Reconstruction from Gravity Using an Auxiliary Field
- Vacuum Solution of a Linear Red-Shift Based Correction in Gravity
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- Propagation and emission of gravitational waves in the weak-field limit within the Palatini formalism